[PDF] Top 20 Clustering and descendants of MUSYC galaxies at z < 1 5
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Clustering and descendants of MUSYC galaxies at z < 1 5
... advantage of features in the spectral energy distribution (SED) to identify sets of galaxies at a particular redshift ...SED at z ∼ 4 and z ∼ 3 (Ouchi et ... See full document
15
XMMU J100750 5+125818: a strong lensing cluster at z = 1 082
... distribution of the cluster member galaxies may point to the principal direction of merging or accretion of XMMU J1007 (Dubinski ...tribution of the brightest member galaxies in ... See full document
8
ALMA Observations of Gas rich Galaxies in z ~ 1 6 Galaxy Clusters: Evidence for Higher Gas Fractions in High density Environments
... taken at face value, this offset implies that star- forming main-sequence galaxies in cluster environments have higher gas masses than the fi ...suggestive of an environmental interaction that ... See full document
6
Lyα emitting Galaxies at z = 2 1 : Stellar Masses, Dust, and Star Formation Histories from Spectral Energy Distribution Fitting
... seen at z 3.1 and are worth studying ...approach of excluding them from SED ...luminosity and limited ...properties and also because number density, EW, luminosity distributions, ... See full document
20
Multiwavelength Study of Massive Galaxies at z~2 I Star Formation and Galaxy Growth
... a 1 00 radius aperture and correlated this measure to the total radio flux density using simulated radio sources of various flux densities (defining an aperture correction, about a factor of ... See full document
17
Heavily Obscured AGN in Star Forming Galaxies at z sime 2
... properties of a sample of individually undetected sources, thus achieving an effective exposure time of many megaseconds ...Miyaji and our own scripts, which are based on CIAO (Fruscione et ... See full document
18
Ly alpha EMITTING GALAXIES AT z=2 1 IN ECDF S: BUILDING BLOCKS OF TYPICAL PRESENT DAY GALAXIES?
... Figure 5 compares the SFRs measured from UV and ...density of objects at the upper left (SFR(UV) > 10 M yr −1 ) and lower left (SFR(UV) < 2 M yr −1 and ... See full document
15
Low ionization galaxies and evolution in a pilot survey up to z = 1
... majority of our individual spectra, which were reduced to zero redshift, have S/N ratios per ...3 at 4200 A. This resolution is very well-adapted to the detec- ˚ tion of small equivalent width [OII] ... See full document
27
Bright strongly lensed galaxies at redshift z similar to 6 7 behind the clusters abell 1703 and CL0024+16
... 2. 5 from the CL0024-iD1 ...are of similar luminosity, differing by only approximately ...Δ z ∼ ...i-dropout and one a z-dropout – at z ∼ ...SEDs, and luminosities, ... See full document
11
Present day descendants of z=3 Ly alpha Emitting galaxies in the millennium II Halo merger trees
... descendant of the more massive central sub-halo. We track the descendants until the two sub-halos merge, possibly triggering star ...timestep of this sub-halo merger and the previous timestep ... See full document
12
PHYSICAL PROPERTIES, STAR FORMATION, AND ACTIVE GALACTIC NUCLEUS ACTIVITY IN BALMER BREAK GALAXIES AT 0 < z < 1
... derivation of the physical properties of 37 Balmer break galaxies, which have the necessary lines to locate them in star-forming–active galactic nuclei (AGNs) diagnostic ...These galaxies span ... See full document
19
Ly alpha emitting galaxies at z=3 1: L* progenitors experiencing rapid star formation
... rest-UV and rest-optical continuua, with mean R-band and ...SED of typical LAEs, which are too dim to be detected individually in our NIR and Spitzer images, we measured av- erage fluxes from ... See full document
7
Introducing the photometric maximum likelihood method: galaxy luminosity functions at z < 1 2 in MUSYC ECDFS
... many of the above criticisms has been suggested more recently by Sheth (2007): the recovered photometric redshift is treated as a quasi-observable distinct from the true redshift, and reproducing its ... See full document
22
The evolution of early type galaxies selected by their spatial clustering
... proposed and applied a new tech- nique, the photometric maximum likelihood (PML) method, to a subset of MUSYC comprising the Extended Chandra Deep Field South (ECDF-S), covering approximately ... See full document
10
The VLT LBG Redshift Survey III The clustering and dynamics of Lyman break galaxies at z similar to 3
... (2008) and Bielby et al. (2011, here- after Paper I), both of whom showed that the clustering evolution of the LBG population may be more complicated, but is likely to produce typical L ... See full document
25
Stellar mass function of cluster galaxies at z ~ 1 5: evidence for reduced quenching efficiency at high redshift
... Adaptation of the Red-Sequence Cluster Survey (SpARCS; Wilson et ...knowledge of the critical phases of galaxy cluster evolution with several z > ...observed and selected in a manner ... See full document
13
The Evolution of Lyα emitting Galaxies between z = 2 1 and z = 3 1
... DENSITY OF LAEs Narrowband imaging (Ouchi et ...2011), and integral-field (Blanc et ...picture of the evolution of the LAE population and their SFR ...luminosities of the ... See full document
11
Ly alpha emission line galaxies at z=3 1 in the extended Chandra Deep Field South
... beam of the Blanco telescope, was computed by combining laboratory measurements of the filter tipped at several different angles from the incoming beam (for a discussion of this procedure, see ... See full document
13
The VLT LBG Redshift Survey I Clustering and dynamics of approximate to 1000 galaxies at z approximate to 3
... models and the Steidel et al. (2003) criteria, we develop a number of selection criteria in the UBR ...R) and to align the (U − B) – (B − R) axis with the stellar locus in the UBR plane, which has a ... See full document
26
The Multiwavelength Survey by Yale Chile (MUSYC): Wide K band imaging, photometric catalogs, clustering, and physical properties of galaxies at z similar to 2
... ( MUSYC ) Wide NIR Survey. The SDSS 1030+05 and Cast 1255 fields were imaged with the Infrared Side Port Im- ager ( ISPI ) on the 4 m Blanco telescope at the Cerro Tololo Inter-American Observatory ... See full document
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